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巻号66
Long-term ...

Long-term variation in the upper atmosphere as seen in the geomagnetic solar quiet daily variation

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Long-term variation in the upper atmosphere as seen in the geomagnetic solar quiet daily variation

国立国会図書館請求記号
Z19-292
国立国会図書館書誌ID
9227909
国立国会図書館永続的識別子
info:ndljp/pid/9227909
資料種別
記事
著者
Atsuki Shinboriほか
出版者
Springer science+business media
出版年
2014-12-11
資料形態
紙・デジタル
掲載誌名
EPS : Earth, Planets and Space 66(155)
掲載ページ
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要約等:

Characteristics of long-term variation in the amplitude of solar quiet (Sq) geomagnetic field daily variation have been investigated using 1-h geomagn...

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デジタル

資料種別
記事
著者・編者
Atsuki Shinbori
Yukinobu Koyama
Masahito Nose
出版年月日等
2014-12-11
出版年(W3CDTF)
2014-12-11
タイトル(掲載誌)
EPS : Earth, Planets and Space
巻号年月日等(掲載誌)
66(155)
掲載巻
66(155)
ISSN(掲載誌)
1880-5981
ISSN-L(掲載誌)
1343-8832
本文の言語コード
eng
国立国会図書館永続的識別子
info:ndljp/pid/9227909
コレクション(共通)
コレクション(障害者向け資料:レベル1)
コレクション(個別)
国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
収集根拠
オンライン資料収集制度
受理日(W3CDTF)
2015-04-17T10:30:12+09:00
保存日(W3CDTF)
2015-02-24
記録形式(IMT)
application/pdf
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国立国会図書館内限定公開
デジタル化資料送信
図書館・個人送信対象外
遠隔複写可否(NDL)
掲載誌(国立国会図書館永続的識別子)
info:ndljp/pid/9227755
連携機関・データベース
国立国会図書館 : 国立国会図書館デジタルコレクション

デジタル

要約等
Characteristics of long-term variation in the amplitude of solar quiet (Sq) geomagnetic field daily variation have been investigated using 1-h geomagnetic field data obtained from 69 geomagnetic observation stations within the period of 1947 to 2013. The Sq amplitude observed at these geomagnetic stations showed a clear dependence on the 10- to 12-year solar activity cycle and tended to be enhanced during each solar maximum phase. The Sq amplitude was the smallest around the minimum of solar cycle 23/24 in 2008 to 2009. The relationship between the solar F10.7 index and Sq amplitude was approximately linear but about 53% of geomagnetic stations showed a weak nonlinear relation to the solar F10.7 index. In order to remove the effect of solar activity seen in the long-term variation of the Sq amplitude, we calculated a linear or second-order fitting curve between the solar F10.7 index and Sq amplitude during 1947 to 2013 and examined the residual Sq amplitude, which is defined as the deviation from the fitting curve. As a result, the majority of trends in the residual Sq amplitude that passed through a trend test showed negative values over a wide region. This tendency was relatively strong in Europe, India, the eastern part of Canada, and New Zealand. The relationship between the magnetic field intensity at 100-km altitude and residual Sq amplitude showed an anti-correlation for about 71% of the geomagnetic stations. Furthermore, the residual Sq amplitude at the equatorial station (Addis Ababa) was anti-correlated with the absolute value of the magnetic field inclination. This implies movement of the equatorial electrojet due to the secular variation of the ambient magnetic field.
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インターネット公開
著作権情報
© 2014 Shinbori et al.; licensee Springer.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.
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連携機関・データベース
国立情報学研究所 : CiNii Research
提供元機関・データベース
学術機関リポジトリデータベース
雑誌記事索引データベース
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書誌ID(NDLBibID)
9227909